activity
20012019
most citedHeating cooling flows with jets

243 citations · 846 across the 9 of their papers we have counts for

collaborators

9 papers

astro-ph.GA2019★ 72 cited

Horizon-AGN virtual observatory - 1. SED-fitting performance and forecasts for future imaging surveys

C. Laigle, I. Davidzon, O. Ilbert +13

Using the ligthcone from the cosmological hydrodynamical simulation Horizon-AGN, we produced a photometric catalogue over with apparent magnitudes in COSMOS, DES, LSST-like…

astro-ph.GA2018★ 61 cited

Galaxies flowing in the oriented saddle frame of the cosmic web

K. Kraljic, C. Pichon, Y. Dubois +12

The strikingly anisotropic large-scale distribution of matter made of an extended network of voids delimited by sheets, themselves segmented by filaments, within which matter flows…

astro-ph.GA2017★ 147 cited

Cosmic evolution of stellar quenching by AGN feedback: clues from the Horizon-AGN simulation

R. S. Beckmann, J. Devriendt, A. Slyz +8

The observed massive end of the galaxy stellar mass function is steeper than its predicted dark matter halo counterpart in the standard CDM paradigm. In this paper, we investiga…

astro-ph.GA2016★ 232 cited

The Horizon-AGN simulation: evolution of galaxy properties over cosmic time

S. Kaviraj, C. Laigle, T. Kimm +6

We compare the predictions of Horizon-AGN, a hydro-dynamical cosmological simulation that uses an adaptive mesh refinement code, to observational data in the redshift range 0<z<6.…

astro-ph.CO2014★ 5 cited

How the cosmic web induces intrinsic alignments of galaxies

Sandrine Codis, Yohan Dubois, Christophe Pichon +2

Intrinsic alignments are believed to be a major source of systematics for future generation of weak gravitational lensing surveys like Euclid or LSST. Direct measurements of the al…

astro-ph.CO2009★ 25 cited

Influence of AGN jets on the magnetized ICM

Y. Dubois, J. Devriendt, A. Slyz +1

Galaxy clusters are the largest structures for which there is observational evidence of a magnetised medium. Central cores seem to host strong magnetic fields ranging from a few 0.…